The southern sky redshift survey

被引:145
|
作者
da Costa, LN
Willmer, CNA
Pellegrini, PS
Chaves, OL
Rite, C
Maia, MAG
Geller, MJ
Latham, DW
Kurtz, MJ
Huchra, JP
Ramella, M
Fairall, AP
Smith, C
Lipari, S
机构
[1] European So Observ, D-85748 Munich, Germany
[2] Observ Nacl, Dept Astron, BR-20921030 Sao Cristovao, RJ, Brazil
[3] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[4] Osserv Astron Trieste, I-34131 Trieste, Italy
[5] Univ Cape Town, Dept Astron, ZA-7735 Rondebosch, South Africa
[6] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA
[7] Observ Astron, RA-5000 Cordoba, Argentina
来源
ASTRONOMICAL JOURNAL | 1998年 / 116卷 / 01期
关键词
galaxies : distances and redshifts; galaxies : photometry;
D O I
10.1086/300410
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report redshifts, magnitudes, and morphological classifications for 5369 galaxies with m(B) less than or equal to 15.5 and for 57 galaxies fainter than this limit, in two regions covering a total of 1.70 sr in the southern celestial hemisphere. The galaxy catalog is drawn primarily from the list of nonstellar objects identified in the Hubble Space Telescope Guide Star Catalog (GSC). The galaxies have positions accurate to similar to 1 " and magnitudes with an rms scatter of similar to 0.3 mag. We compute magnitudes (m(SSRS2)) from the relation between instrumental GSC magnitudes and the photometry by Lauberts & Valentijn. From a comparison with CCD photometry, we find that our system is homogeneous across the sky and corresponds to magnitudes measured at the isophotal level similar to 26 mag arcsec(-2). The precision of the radial velocities is similar to 40 km s(-1), and the redshift survey is more than 99% complete to the m(SSRS2) = 15.5 mag limit. This sample is in the direction opposite that of the CfA2; in combination the two surveys provide an important database for studies of the properties of galaxies and their large-scale distribution in the nearby universe.
引用
收藏
页码:1 / 7
页数:7
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